Star Obsession
Star Obsession is a 3-year-old still searching for a breakthrough after four races without a win or a place. The horse's recent form reads 8-4-4-5 (most recent first), showing some promise in the middle two races but nothing yet to suggest a maiden victory is imminent. At Class 4 level—the lower rungs of British racing—Star Obsession has tried three times without success, finishing unplaced each time.Based on TrackLab's analysis
📊 Key numbers
Career totals for this horse
🔍 Full analysis
Our model's view, based on this horse's career and recent runs
The horse is trained by William Haggas at Newmarket, one of the sport's most respected operations. Haggas's yard has already sent out 170 winners this season, so Star Obsession is in a capable setup. Still, raw ability and opportunity alone do not guarantee results, and this horse has yet to find the right conditions or race to deliver. With racing happening at pace and Star Obsession active just yesterday, answers about whether this horse has what it takes may not be far away.
🎯 Where this horse runs best
Results split by ground, distance, race level and track shape
🌧 Ground
Standard to slow (all-weather)
Unknown
Standard (all-weather)
Unknown
Good to firm (fairly firm)
Unknown
🏅 Race level
Class 4 (standard)
Unknown
🏟 Track shape
Right-handed, long straights
Unknown
Left-handed, long straights
Unknown
Right-handed, tight turns
Unknown
📅 Recent runs
The last 10 races, most recent first
24 Aug
8th
Windsor
5f – 6½f · Good_To_Firm · 9 runners
11 Feb
4th
Kempton Park
1m1f – 1m2f · Standard_To_Slow · 8 runners
4 Feb
4th
Kempton Park
1m1f – 1m2f · Standard_To_Slow · 12 runners
2 Jan
5th
Wolverhampton
7f – 1m · Standard · 8 runners
🏇 Jockeys
Every jockey who has ridden this horse, most rides first
🏟 Course record
Win rate at each course this horse has visited
| Course | Races | Results | Last run | Win rate |
|---|
| Kempton Park Galloping |
2 |
2 other |
11 Feb |
0% |
| Wolverhampton Galloping |
1 |
1 other |
2 Jan |
0% |
| Windsor Sharp |
1 |
1 other |
24 Aug |
0% |